SDO HMI 2014-11-29 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.01 | 26.07 | 4.27 | 15.55 | 16.75 | 152.28 | 30.52 | 299.28 | 0.5596 | 108.2 | -70.9 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.13 | 7.53 | 3.15 | 4.61 | 17.35 | 154.54 | 32.78 | 298.68 | 0.5913 | 851.1 | 611.5 | |
| 1.11 | 2.05 | 0.66 | 1.22 | 15.37 | 152.76 | 31.00 | 296.64 | 0.5577 | 824.7 | 731.6 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 15.13 | 152.61 | 30.85 | 296.33 | 0.5545 | 785.0 | 628.1 | |
| 0.77 | 2.39 | 0.46 | 1.42 | 15.68 | 152.17 | 30.41 | 297.56 | 0.5518 | 845.4 | 698.1 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 16.51 | 152.20 | 30.44 | 298.91 | 0.5571 | 704.0 | 597.7 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 15.56 | 152.04 | 30.28 | 297.44 | 0.5495 | 769.0 | 452.9 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 17.23 | 151.15 | 29.39 | 300.86 | 0.5482 | -739.0 | -647.5 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 17.26 | 151.05 | 29.29 | 300.99 | 0.5471 | -598.0 | -443.6 | |
| 0.00 | 1.37 | 0.00 | 0.81 | 17.48 | 150.66 | 28.90 | 301.66 | 0.5437 | -549.0 | -460.1 | |
| 0.00 | 2.48 | 0.00 | 1.45 | 16.53 | 150.46 | 28.70 | 300.22 | 0.5350 | -858.0 | -696.2 | |
| 0.00 | 1.37 | 0.00 | 0.80 | 17.45 | 150.48 | 28.72 | 301.76 | 0.5412 | -729.0 | -654.8 | |
| 0.00 | 2.65 | 0.00 | 1.55 | 17.18 | 150.29 | 28.53 | 301.45 | 0.5370 | -839.0 | -732.0 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 17.89 | 150.38 | 28.62 | 302.55 | 0.5429 | -754.0 | -702.9 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |